SA43A-2359
LASER MEASUREMENTS OF THE H ATOM + OZONE RATE CONSTANT AT ATMOSPHERIC TEMPERATURES
Thursday, 17 December 2015
Poster Hall (Moscone South)
Gregory P Smith1, Yingdi Liu1, Jian Peng1, Kelsey James Reppert2 and Sara Lynn Callahan3, (1)SRI International Menlo Park, Menlo Park, CA, United States, (2)North Carolina State University Raleigh, Raleigh, NC, United States, (3)Organization Not Listed, Washington, DC, United States
Abstract:
The exothermic H + O3 reaction produces OH(v) Meinel band emissions, used to derive mesospheric H concentrations and chemical heating rates. We have remeasured its rate constant to reduce resulting uncertainties and the measurement extend to lower mesospheric temperatures using modern laser techniques. H atoms are produced by pulsed ultraviolet laser trace photolysis of O3, followed by reaction of O(D) with added H2. A second, delayed, frequency-mixed dye laser measures the reaction decay rate with the remaining ozone by laser induced fluorescence. We monitor either the H atom decay by 2 photon excitation at 205 nm and detection of red fluorescence, or the OH(v=9) product time evolution with excitation of the B-X (0,9) band at 237 nm and emission in blue B-A bands. By cooling the enclosed low pressure flow cell we obtained measurements from 146-305 K. Small kinetic modeling corrections are made for secondary regeneration of H atoms. The results fully confirm the current NASA JPL recommendation for this rate constant, and establish its extrapolation down to the lower temperatures of the mesosphere. This work was supported by the NSF Aeronomy Program and an NSF Physics summer REU student grant.